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Hello, I get an error when running the program "ERROR: can't read default.nnw".
I found on internet somewhere advice to transfer the default.nnw from config directory in the program, to my working di…
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Is anyone working on extending lightkurve to accept the TESS PRF? If not I'll try to make that work. I need this capability ASAP to do pixel-level transit modeling for TESS false positive identifica…
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# TODO before submitting
- [x] Attach or link a logo (preferably square, no background)
- If no logo is available then instead write that in a comment and change the data to have `"logo": ""` …
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The `stitch()` function throws a ton of new `MergeConflictWarnings`. I've included an example below.
```python3
collection = search_result[0:2].download_all()
collection.stitch()
WARNING: Merg…
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### Description
Forgive me but I think the year given between authors and abstract in HTML differs from the year given above the title, 2022 vs 2024.
### (Optional:) Please add any files, screenshot…
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![249200379 - 14 - MS - Echelle](https://github.com/user-attachments/assets/22ba1b0d-8966-455c-9270-3cf60dcbce01)
![249200379 - 14 - MS - Mode ID](https://github.com/user-attachments/assets/a57110d7-…
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Is it possible to read a fits light curve from other missions like Swift?. Those files basically have time, rate and error as columns and some info in the header. I would like to be able to read it …
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I recently had another look at f3 and wondered about conceivable extensions and applications.
### Is it possible to calibrate the C5, C16, C18 FFIs in the same way as the Kepler prime mission?
As…
gully updated
5 years ago
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Hey folks! I've given your JOSS text a close read, and I have a few suggestions based on the checkbox items of the JOSS review process. I'm a total astroseismology noob, so please forgive my ignorance…
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------------ ISSUE 1 ---------------------
The standard format for `tr.spacetime_lookup` given in the example notebook:
`ra = 249.82602
dec = 66.22553
obs = tr.spacetime_lookup(ra=ra,dec=dec)`
…